Recurring Homologous Solar Eruptions in NOAA AR 11429
Suman K. Dhakal, Jie Zhang, Panditi Vemareddy, Nishu Karna

TL;DR
This study analyzes three recurrent solar eruptions from NOAA AR 11429, highlighting the roles of magnetic flux cancellation, shearing motions, and magnetic topology in driving homologous eruptions over several days.
Contribution
It provides new insights into the physical processes behind recurrent homologous eruptions, emphasizing the importance of flux cancellation and magnetic topology in eruption mechanisms.
Findings
Persistent flux cancellation leads to recurrent eruptions.
Magnetic flux rope formation and reformation occur along the same PIL.
Magnetic reconnection at the same location facilitates eruptions.
Abstract
We present the study of three homologous solar eruptions from NOAA active region (AR) 11429 over four days. This large and complex AR divided into two relatively simple sub-regions: northeast (NE) and southwest (SW). Recurrent eruptions occurred from the SW sub-region over different evolutionary phases, which provided a unique opportunity to isolate the physical processes responsible for solar eruptions. Persistent shearing and convergence of opposite magnetic polarities led to continuous flux cancellation along the SW polarity inversion line (PIL). A filament persistently lying along the SW-PIL was observed to survive each eruption, which suggests the partial eruption of the magnetic system. Further, following the first and second eruptions, a sigmoidal magnetic structure of similar morphology was reformed along the SW-PIL. The photospheric motion of magnetic flux continuously injected…
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